Vacuum thin shell solutions in five-dimensional Lovelock gravity
Abstract
Junction conditions for vacuum solutions in five-dimensional Einstein-Gauss-Bonnet gravity are studied. We focus on those cases where two spherically symmetric regions of space-time are joined in such a way that the induced stress tensor on the junction surface vanishes. So a spherical vacuum shell, containing no matter, arises as a boundary between two regions of the space-time. Such solutions are a generalized kind of spherically symmetric empty space solutions, described by metric functions of the class . New global structures arise with surprising features. In particular, we show that vacuum spherically symmetric wormholes do exist in this theory. These can be regarded as gravitational solitons, which connect two asymptotically (Anti) de-Sitter spaces with different masses and/or different effective cosmological constants. We prove the existence of both static and dynamical solutions and discuss their (in)stability under perturbations that preserve the symmetry. This leads us to discuss a new type of instability that arises in five-dimensional Lovelock theory of gravity for certain values of the coupling of the Gauss-Bonnet term.
Cite
@article{arxiv.1001.3096,
title = {Vacuum thin shell solutions in five-dimensional Lovelock gravity},
author = {C. Garraffo and G. Giribet and E. Gravanis and S. Willison},
journal= {arXiv preprint arXiv:1001.3096},
year = {2010}
}
Comments
9 pages. This is an extended version of the authors' contribution to the Proceedings of the Marcel Grossmann Meeting, held in Paris, 12-18 July 2009